188
Müller und Kempf, Photometrische Durchmusterung
188
K.D.
Sternzeit
I
II
III
IV
J
■r
logsin 2 «/
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 157. 1887 Juni 7.
Beobachter: Kempf.
Photometer: D. Vergleichsterne: Nr. 30
und Nr. 3
2. Luft:
>— 4 -
8 0 28 57
1 5 li 37 m
2786
2785
3089
28%
28865
4 6? 5
9-3615
9.3998
II 2780
15 40
22.2
23-5
24.1
234
23-3°
41.8
9.1944
9.2221
I 2941
15 42
27.0
29.0
30.6
28.5
28.78
53-6
9-3651
9.4260
0.1024
— O.26
6.19
5 2886
15 44
25.6
26.5
28.2
27-5
26.95
49.8
9.3126
9.3602
0.0366
— O.09
6.36
4 2878
15 45
15-3
15.8
18.5
16.3
16.48
50.3
8.9057
8.9548
O.3688
+ O.92
7-37
5 2889
15 47
16.8
17-5
19-5
18.1
17.98
49.4
8.9791
9-0255
0.2981
+ 0.75
7.20
2 2844
15 48
20.0
20.6
24.0
22.5
21.78
52.0
9.1388
9- 1 93 7
O.1299
+ O.32
6.77
0 3223
15 51
9.8
10.0
12.5
1 1-3
10.90
54 -i
8-5534
8.6163
0.7073
+ i -77
8.22
8 2857
15 53
24.9
28.0
33 -o
30.5
29.10
47-7
9-3739
9.4154
11 2780
15 55
23.8
24.6
24-5
24.2
24.28
424
9.2281
9.2570
1 2972
15 58
29.0
28.2
324
30.1
29.92
53-7
9-3958
9 - 457 1
0.1335
— 0.33
6.12
8 2914
15 59
17.0
17.0
16.6
18.5
17.28
46.7
8.9456
8.9844
0.3392
+ 0.85
7-30
1 2981
16 1
16.9
16.9
20.5
18.9
18.30
53-6
8.9938
9-0547
0.2689
—j— 0.67
7.12
6 2946
16 3
17*5
18.2
21.1
19.0
18.95
48.8
9.0231
9.0677
0.2559
~b 0.64
7.09
8 2925
16 4
17.1
17.6
21.0
19.1
18.70
46.8
9.0120
9.0511
0.2725
-b 0.68
7-13
0 3253
16 6
23-5
24.1
27.0
26.4
25-25
54-9
9.2600
9-3263
0.0027
— 0.01
6-44
Mittel aus den
Vergleichsternbeobachtungen: 9.3110; 9.3362. Zur Reduction benutzt: 9.3236.
Die Beobachtungen
der Vergleichsterne
am Schluss der Zone wurden durch
plötzliche Wolkenbildung ver-
hindert. Die übrigen
Messungen scheinen einwurfsfrei.
Zone 158. 1887 October 12.
Beobachter : Kempf.
Photometer :
D. Vergleichsterne: Nr. 46 und Nr. 48. Luft:
2.
9° 5 111
2i b 59 ra
2 i?o
230
2487
20?9
22852
4385
9.1664
9.1976
9 5277
22 2
21-5
19.7
21.1
22.0
21.08
47.2
9.1118
9 -I 5 I 9
O 4950
22 4
34-5
33-6
35-5
324
34.02
53 -o
9.4956
9-5542
0.4100
— 1.03
5-73
4 4935
22 6
18.7
16.0
19-5
I7.6
17-95
48.9
8.9777
9.0226
O.12 16
+ 0.30
7.06
2 4594
22 8
31-0
28.5
29.0
27.7
29.05
50.9
9-3725
9.4236
O.2794
— 0.70
6.06
3 4814
22 IO
17.0
15.0
174
16.5
16.48
49-5
8.9057
8.9524
0.1918
+ 0.48
7.24
2 4597
22 11
22.9
22.0
22.6
22.2
22.42
504
9.1627
9.2122
0.0680
— 0.17
6-59
5 5123
22 13
20.5,
21.5
234
22-5
21.98
47-3
9.1464
9.1868
O.0426
O.I I
6.65
9 5111
22 15
20.4
20.0
20.4
20.4
20.30
42.9
9.0805
9.1104
9 5277
22 17
21.2
19.0
22.4
20.5
20.78
46.0
9.0999
9 -Ì 369
0 4963
22 20
20.4
21.9
21.7
20.3
21.08
52-4
9.1118
9.1682
0.0240
— 0.06
6.70
1 4686
22 23
34 -o
37 - 1
33-1
37 - 6
35-45
51.6
9.5269
9.5804
O.4362
— 1.09
5-67
6 5124
22 25
14.7
14.6
16.0
15.0
15.08
46.3
8.8305
8.8683
O.2759
-b 0.69
7-45
4 4975
22 27
21-5
22.6
23-5
23.0
22.65
48.7
9.1712
9-2155
O.0713
— 0.18
6.58
4 4985
22 28
15.2
16.9
18.8
16.2
16.78
48.7
8.9209
8.9652
0.1790
+ 0.45
7.21
7 499 1
22 .30
38.1
40.3
42.8
38.0
39.80
44.9
9.6125
9.6469
0.5027
—1.26
5-50
9 51“
22 32
21.5
21.1
19-5
19.9
20.50
42.6
9.0887
9.1180
9 5277
22 34
20.5
21.5
23-3
19-5
21.20
44.8
9-1165
9 - I 5°6
Mittel aus den Vergleichsternbeobachtungen: 9.1748
; 9.1236; 9.1343. Zur Reduction benutzt: 9.1442.
Zone 15g
. 1887 October 12.
Beobachter : Müller.
Photometer :
D. Vergleichsterne: Nr. 46 und Nr. 48. Luft:
2.
9 ° 5 2 7 7
22 h 36™
19?6
i 8?3
1987
i8?o
18890
4487
9.0209
9.0548
9 5 111
22 40
21.6
18.9
21-5
18.5
20.12
42-5
9 - 073 I
9.1022
5 5150
22 42
10.9
10.3
II 4
9-5
10.52
47.1
8.5229
8.5628
0.5283
+ 1-32
8.08
7 5009
22 45
17.4
14.6
17.O
1 7-7
16.68
454
8.9159
8.9515
0.1396
+ 0.35
7.n
8 5058
22 49
11.6
11-3
14-3
12.3
12.38
44-5
8.6624
8.6958
0.3953
+ 0.99
7-75
7 5030
22 51
15.0
14.0
15.6
14.7
14.82
44-8
8.8157
8.8498
0.2413
-b 0.60
7-36
0 4999
22 53
22.5
23-4
25-3
21.8
23-25
52.2
9.1927
9.2483
0.1572
— 0.39
6-37
4 5 ° l6
22 54
17.7
13-7
15.0
13.8
I 5-05
48.4
8.8288
8.8723
0.2 l88
+ 0.55
7-31
9 5111
22 56
20.5
19.4
21.0
17.7
19.65
42.6
9-0534
9.0827
